Optical photometry and spectroscopy of Nova Del 2013
Abstract
We report optical BV photometry and spectroscopy of Nova Del 2013, carried out between August 14.88 UT and August 15.08 UT. Using a 60 cm Cassegrain telescope at the Nicolaus Copernicus University Observatory (Torun, Poland) we estimated the V brightness of the Nova to be 6.31+/-0.02 mag and 6.18+/-0.03 mag on Aug. 14.94 UT and Aug. 15.02 UT respectively. HD 194113 (F2, V=8.00 mag) was used as a comparison star.
- Publication:
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The Astronomer's Telegram
- Pub Date:
- August 2013
- Bibcode:
- 2013ATel.5288....1T
- Keywords:
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- Optical;
- Nova